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Water induced sediment levitation enhances downslope transport on Mars

On Mars, locally warm surface temperatures (~293 K) occur, leading to the possibility of (transient) liquid water on the surface. However, water exposed to the martian atmosphere will boil, and the sediment transport capacity of such unstable water is not well understood. Here, we present laboratory...

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Detalhes bibliográficos
Publicado no:Nat Commun
Main Authors: Raack, Jan, Conway, Susan J., Herny, Clémence, Balme, Matthew R., Carpy, Sabrina, Patel, Manish R.
Formato: Artigo
Idioma:Inglês
Publicado em: Nature Publishing Group UK 2017
Assuntos:
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC5658360/
https://ncbi.nlm.nih.gov/pubmed/29075001
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41467-017-01213-z
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